2.2k citations · 36.2k across the 274 of their papers we have counts for
273 papers
WISDOM project -- XXIII. Star-formation efficiencies of eight early-type galaxies and bulges observed with SITELLE and ALMA
Anan Lu, Daryl Haggard, Martin Bureau +18
Early-type galaxies (ETGs) are known to harbour dense spheroids of stars with scarce star formation (SF). Approximately a quarter of these galaxies have rich molecular gas reservoi…
WISDOM Project -- XXII. A 5% precision CO-dynamical supermassive black hole mass measurement in the galaxy NGC 383
Hengyue Zhang, Martin Bureau, Ilaria Ruffa +8
We present a measurement of the supermassive black hole (SMBH) mass of the nearby lenticular galaxy NGC 383, based on Atacama Large Millimeter/sub-millimeter Array (ALMA) observati…
WISDOM Project -- XXI. Giant molecular clouds in the central region of the barred spiral galaxy NGC 613: a steep size -- linewidth relation
Woorak Choi, Martin Bureau, Lijie Liu +9
NGC~613 is a nearby barred spiral galaxy with a nuclear ring. Exploiting high spatial resolution ( pc) Atacama Large Millimeter/sub-millimeter Array CO(1-0) obser…
WISDOM Project -- XIX. Figures of merit for supermassive black hole mass measurements using molecular gas and/or megamaser kinematics
Hengyue Zhang, Martin Bureau, Mark D. Smith +7
The mass () of a supermassive black hole (SMBH) can be measured using spatially-resolved kinematics of the region where the SMBH dominates gravitationally. The most…
WISDOM Project -- XXVI. Cross-checking supermassive black hole mass estimates from ALMA CO gas kinematics and SINFONI stellar kinematics in the galaxy NGC 4751
Pandora Dominiak, Michele Cappellari, Martin Bureau +6
We present high angular resolution ( or pc) ALMA observations of the CO(3-2) line emission of the galaxy NGC 4751. The data provide evidence for the pres…
SDSS-IV MaNGA: Calibration of astrophysical line-widths in the Hα region using HexPak observations
Sabyasachi Chattopadhyay, Matthew A. Bershady, David R. Law +7
We have re-observed 40 low-inclination, star-forming galaxies from the MaNGA survey ($\upsigma\sim65$~\kms) at 6.5 times higher spectral resolution ($\upsigma\sim10$…